Synthetic images of the simulated disk at 0° inclination. The top row shows the brightness of the simulated disk after radiative transfer for four different ALMA wavelength bands (columns). The bottom row shows the convolution of the disk images using a circular beam with a FWHM of 12 au (σ_beam = 5 au). Overall, the presence of two asymmetric dust features are clearly seen at the inner ring and in the outer parts of the dust continuum emission. The inner one was found to be at the same location as the dust concentration.